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Cosmogenic neutrino production from the propagation of ultra-high energy cosmic-ray nuclei

D. Allard 1
1 APC - AHE - APC - Astrophysique des Hautes Energies
APC (UMR_7164) - AstroParticule et Cosmologie, Dipartimento di Astronomia, Universita degli Studi di Bologna
Abstract : In this proceeding, we study the production of cosmogenic neutrinos from the propagation of ultra-high energy cosmic-ray (UHECR) nuclei. After discussing the main production channels for cosmic-ray nuclei, we investigate the dependence of the expected fluxes on astrophysical parameter such as the composition, the cosmological distribution of the sources, or the maximum energy of the accelerated cosmic-rays. We finally discuss the detectability of these cosmogenic neutrinos between 10^12 and 10^20 eV.
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http://hal.in2p3.fr/in2p3-00372092
Contributor : Simone Lantz <>
Submitted on : Tuesday, March 31, 2009 - 11:54:11 AM
Last modification on : Friday, October 30, 2020 - 12:04:03 PM

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D. Allard. Cosmogenic neutrino production from the propagation of ultra-high energy cosmic-ray nuclei. Neutrino Oscillation Workshop - NOW 2008, Sep 2008, Conca Specchiulla, Oranto, Italy. pp.293-296, ⟨10.1016/j.nuclphysbps.2009.02.069⟩. ⟨in2p3-00372092⟩

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